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Table 1:

Log of the observationsa.
Date Days to $\Delta$ $R_{\rm S}$ $m_{\rm v}$ Alpha Sun-C Telescope D Filters Exposure
2008-2009 perihelion (AU) (AU)   ($^{\circ }$) PA ($^{\circ }$)   ( km px-1)   time
December                    
25.60 -65 1.67 1.45 14.2 35.75 70.5   370 CR 180 s
26.62 -64 1.67 1.46 14.2 35.75 70.5 IGO 373 CR 120 s $\times$ 2
27.59 -63 1.67 1.46 14.2 35.8 70.4 (India) 373 CB 240 s $\times$ 2
27.61 -63 1.67 1.46 14.2 35.8 70.3 2 m 373 CR 180 s $\times$ 2
27.63 -63 1.67 1.46 14.2 35.8 70.3   373 $R_{\rm b}$ 60 s $\times$ 2
March                    
17.81 +17 1.72 1.26 13.5 34.7 69.9 OHP 1051 R 20 s $\times$ 9
18.78 +18 1.72 1.265 13.5 34.7 70.0 (France) 1057 R 20 s $\times$ 18
19.80 +19 1.73 1.27 13.5 34.6 70.2 0.8m 1057 R 20 s $\times$ 21
April-May                    
30.60 +61 1.99 1.44 14.5 28.9 82.3 IGO 445 R$_{\rm b}$ 360 s
01.70 +62 2.00 1.45 14.5 28.7 82.7 2 m 445 R$_{\rm b}$ 600 s

Notes. (a) $\Delta$ = Earth-comet distance; $R_{\rm S}$ = Sun-comet distance; $m_{\rm v}$ = expected magnitudes given by the JPL Horizons system ephemeris; $\alpha$ = phase angle; Sun-C PA = extended Sun-comet radius vector position angle; D = projected diameter for 1 pixel; filters: CR = narrow cometary red filter, CB = narrow cometary blue filter, $R_{\rm b}$ = broad red filter centered on 620 nm, R = broad red filter centered on 650 nm (see Sect. 2.1). Exposure time for each polarized component image $\times$ number of images used for the results.


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